Entropy of Thermally Excited Black Rings
arXiv:hep-th/0505152 · doi:10.1088/1126-6708/2005/10/100
Abstract
A string theory description of near extremal black rings is proposed. The entropy is computed and the thermodynamic properties are derived for a large family of black rings that have not yet been constructed in supergravity. It is also argued that the most general black ring in N=8 supergravity has 21 parameters up to duality.
17 pages; v2: minor edits and refs added
References in corpus (8)
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Cited by in corpus (21)
- Black Holes in Higher Dimensions
- Bubbling Supertubes and Foaming Black Holes
- Black Rings
- Bicycling Black Rings
- Universal properties and the first law of black hole inner mechanics
- Quasilocal Formalism and Black Ring Thermodynamics
- The Role of Dipole Charges in Black Hole Thermodynamics
- Black holes in N=8 supergravity from SO(4,4) hidden symmetries
- A (Running) Bolt for New Reasons
- Extremal solutions of the S3 model and nilpotent orbits of G2(2)
- Holographic Descriptions of Black Rings
- A General Black String and its Microscopics
- Generating technique for supergravity
- Black Holes with Intrinsic Spin
- A Charged Doubly Spinning Black Ring
- Three-charge 2J black ring
- On Black Ring with a Positive Cosmological Constant
- Exact Microscopic Entropy of Non-Supersymmetric Extremal Black Rings
- Constructing near-horizon geometries in supergravities with hidden symmetry
- Note on the thermodynamic stability of a black ring at quantum scales
- Entanglement entropy for non-zero genus topologies